Robert Raynolds McMath
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American astronomer
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Why Is Robert Raynolds McMath Influential?
(Suggest an Edit or Addition)According to Wikipedia, Robert Raynolds McMath was an American solar astronomer. McMath was a bridge engineer, businessman, and astronomer. His father, Francis C. McMath, had made a fortune as a bridge builder. They both had a keen interest in amateur astronomy. So in 1922, the McMaths, along with Judge Henry S. Hulbert founded the McMath–Hulbert Observatory in Lake Angelus, Michigan. It was deeded to the University of Michigan in 1931, McMath served as the director of the McMath–Hulbert Observatory until 1961.
Robert Raynolds McMath's Published Works
Number of citations in a given year to any of this author's works
Total number of citations to an author for the works they published in a given year. This highlights publication of the most important work(s) by the author
Published Works
- Preliminary Results with a Vacuum Solar Spectrograph. (1956) (22)
- SOLAR FEATURES ASSOCIATED WITH ELLERMAN'S "SOLAR HYDROGEN BOMBS". (1960) (22)
- Photometry of Solar Flares. (1956) (20)
- Observations of Solar Limb Darkening Between 0.5 and 10.2&mu (1950) (15)
- Solar Spectroscopy with a Vacuum Spectrograph. (1956) (11)
- Carbon Dioxide in the Infra-Red Solar Spectrum (1949) (10)
- Telluric Bands of CH_{4} in the Solar Spectrum. (1949) (10)
- Solar Spectroscopy with a Cashman Cell (1949) (9)
- The Limb Flare of may 8, 1951. (1951) (9)
- No. 568. Prominences of the active and sun-spot types compared. (1937) (7)
- Solar spectroscopy with echelles. (1951) (7)
- Table of Infrared Solar Lines, 1.4-2.5 μ. (1953) (6)
- Identification of CO in the Solar Atmosphere (1952) (5)
- New Solar Lines in the Spectral Region 1.52-1.75 μ. (1949) (5)
- Telluric Bands of Methane in the Fraunhofer Spectrum (1948) (5)
- N 2 O Bands in the Solar Spectrum (1950) (5)
- Isotopes of Carbon and Oxygen in the Earth's Atmosphere (1948) (4)
- THE DOPPLER EFFECT IN AN ERUPTIVE PROMINENCE (1939) (4)
- Doppler Shifts in Solar Granules. (1955) (4)
- The Abundance of CO in the Sun and in the Earth's Atmosphere (1952) (4)
- Motion pictures of small chromospheric flocculi (1939) (4)
- An Experimental Study of Fretting Wear in Gear Tooth Flexible Couplings (1961) (4)
- New Solar Lines in the Spectral Region 1.97-2.49 μ. (1950) (3)
- The Abundance and Temperature of Methane in the Earth's Atmosphere (1948) (3)
- Spectroscopic Evidence for Ammonia in the Earth's Atmosphere (1948) (3)
- AN ERUPTIVE PROMINENCE OF RECORD HEIGHT AND VELOCITY (1937) (2)
- Tower Telescopes and Accessories (1953) (2)
- Simultaneous observations of solar flares, surges, and high-speed dark flocculi (1948) (2)
- HIGH-DISPERSION SOLAR SPECTRUM IN THE 10,000 A TO 20,000 A REGION (1947) (2)
- Note on Methane in the Infra-Red Solar Spectrum (1949) (2)
- A General Study of a Prominence Field (1948) (2)
- New Atomic Lines in the Infra-Red Solar Spectrum (1947) (1)
- NEW BANDS IN THE TELLURIC SPECTRUM (1948) (1)
- The McGregor Building and Tower Telescope of the McMath-Hulbert Observatory (1940) (1)
- Excited-State Bands of Atmospheric CO2 (1949) (1)
- SOME NEW PROMINENCE PHENOMENA (1937) (1)
- LOCATION OF VELOCITY CHANGES IN A CLASS IIIB PROMINENCE (1939) (1)
- MOTIONS IN THE LOOPS OF PROMINENCES OF THE SUNSPOT TYPE, CLASS III B (1938) (1)
- SOLAR RESEARCH AT THE MCMATH-HULBERT OBSERVATORY (1952) (0)
- Artificial Limbs (1945) (0)
- The new solar tower of the McMath-Hulbert Observatory (1936) (0)
- HYPERVELOCITY PARTICLE EFFECTS ON MATERIAL (1962) (0)
- The Large Solar Telescope at Kitt Peak II (1960) (0)
- The 50-foot focal length vacuum spectrograph for solar research. (1954) (0)
- The Francis C. McMath memorial 24-inch reflecting telescope of the McMath-Hulbert Observatory (1943) (0)
- A QUASI-ERUPTIVE PROMINENCE OBSERVED IN HYDROGEN (1938) (0)
- A reflecting spectrometer for the solar infra-red. (1948) (0)
- SOLAR FILAMENT OF SEPTEMBER 7, 1948 (1948) (0)
- Photometric studies of solar flares. (1951) (0)
- Telescope Driving Mechanisms (1961) (0)
- A Solar Infrared Reflecting Spectrometer (1948) (0)
- The Surface of the Nearest Star (1939) (0)
- Problems of the Infrared Solar Spectrum (1949) (0)
- The McMath-Hulbert telechron driving-clock (0)
- Evidence for coronal absorption on the solar disk. (1947) (0)
- Clouds Partially Veil Eclipse; Observers Win against Odds (1932) (0)
- ATTENUATION OF POINT SOURCE GAMMA RADIATION IN SLABS. Final Report (1962) (0)
- Recent developments in infra-red solar spectroscopy. (1948) (0)
- The3ν3-Band of Telluric CO2in the Solar Spectrum (1950) (0)
- The use of a high dispersion spectrograph in the wave-length region 1.0 to 2.0 microns. (1948) (0)
- A report on the solar prominence radial velocity program of the McMath-Hulbert Observatory (1946) (0)
- RESULTS AND ANALYSIS OF ROOM TEMPERATURE PRESSURE TESTING OF THE HOWARD FOUNDRY PESCO PUMP VOLUTE S-2463-1 PWA #248773 (1957) (0)
- The measurement of space motions of solar prominences (1943) (0)
- The 3n3 Band of Telluric CO 2 in the Solar Spectrum (1950) (0)
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